Fig. 11
SCExAO/VAMPIRES images of Procyon A at 750 nm before (left) and after (right) our focal plane closed-loop wavefront control on the IE. A 0.5 power scale is used to represent these frames. Each image is normalized to its intensity peak and both frames are represented with a different color scale to enhance the image differences between them. The star image is sharper after IE compensation.
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